A test of general relativity using radio links with the Cassini spacecraft
By B. Bertotti, L. Iess, P. Tortora. Nature, 2003
1,770 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/ef8395964a6b17068d49b6c71344e30ae0c019c1
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In Astronomy and Astrophysics
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In Nuclear and High Energy Physics
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Citations in the corpus
- Relativistic effects and solar oblateness from radar observations of planets and spacecraft (2005, methodology): “Some of the recent post-Newtonian-parameter 1063-7737/05/3105-0340$26.00 c© 2005 Pleiades Publishing, Inc. determinations, e.g., γ = 1.000021 ±0.000023, from Cassini radar observations (Bertotti et al. 2003) reach a high accuracy.”
- Effective field theory of dark energy: A review (2019, background): “The theory is very well constrained at all scales: ωBD > 4 × 10(4) from Shapiro time delay [255], ωBD > 6 × 10(2) from Planck [256].”
- A 2.1 M☉ Pulsar Measured by Relativistic Orbital Decay (2005, background): “BD > 40;000, from radio ranging to the Cassini probe (Bertotti et al. 2003).”
- Higher Order Gravity Theories and Their Black Hole Solutions (2008, methodology): “Most stringent constraints arise from light time delay which is calculated from the Cassini spacecraft [75].”